Methods of Celestial Mechanics: Volume II: Application to Planetary System, Geodynamics and Satellite GeodesySpringer Science & Business Media, 21.11.2005 - 448 Seiten G. Beutler's Methods of Celestial Mechanics is a coherent textbook for students as well as an excellent reference for practitioners. The first volume gives a thorough treatment of celestial mechanics and presents all the necessary mathematical details that a professional would need. The reader will appreciate the well-written chapters on numerical solution techniques for ordinary differential equations, as well as that on orbit determination. In the second volume applications to the rotation of earth and moon, to artificial earth satellites and to the planetary system are presented. The author addresses all aspects that are of importance in high-tech applications, such as the detailed gravitational fields of all planets and the earth, the oblateness of the earth, the radiation pressure and the atmospheric drag. The concluding part of this monumental treatise explains and details state-of-the-art professional and thoroughly-tested software for celestial mechanics. |
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... in the system J2000.0 Arg. of Perigee Long. of Perigee Fig. 2.15. Amplitude spectrum. 4.95 1980 1985 1990 1995 2000 2005 2010 2015 2020 2025 Year incl - 1 W – W = – (~ cos 694. 2.2 The Rotation of a Rigid Earth and a Rigid Moon 27.
... spectrum of the type shown in Figure 2.15. The contributing elements of the spectrum to such a line have to be added in a mathematically correct way – as described in Chapter 11 of Part III. The result is contained in Table 2.3. 01 2 3 ...
... spectrum is dominated by a few prominent lines, which were discovered empirically a long time ago: 1. Equation of ... spectrum of the. Fig. 2.15. Amplitude spectrum of the ecliptical longitude of the Moon (de-trended) using a 400-years ...
... spectrum of the lunar ecliptical longitude∗ Name Period (theor.) Period (spectrum) Amp [ days ] [◦] Equation of Center 2 π/n 27.5581 6.2815 Evection 2 π /( 2(nω − n⊙) + n ) 31.8230 1.2759 /( ) Variation 2π 2(n − n⊙) 14.7670 0.6638 ...
... Fig. 2.18. Euler angles Ψ♁, ε♁ and Θ♁ (minus mean motion) at beginning of 1981 without torques Fig. 2.20. Spectrum of the Oppolzer motion Fig. 2.21. Precession. 2.2 The Rotation of a Rigid Earth and a Rigid Moon 37.
Inhalt
3 | |
6 | |
14 | |
Artificial Earth Satellites | 123 |
Evolution of the Planetary System | 211 |
Variational Equations | 272 |
5 | 301 |
The ComputerPrograms NUMINT and LINEAR | 311 |
The ComputerPrograms SATORB and LEOKIN | 323 |
The ComputerProgram ORBDET 355 | 354 |
The ComputerProgram ERDROT | 371 |
The ComputerProgram PLASYS | 387 |
Elements of Spectral Analysis | 394 |
References | 425 |
Abbreviations and Acronyms 433 | 432 |
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Methods of Celestial Mechanics: Volume II: Application to Planetary System ... Gerhard Beutler Eingeschränkte Leseprobe - 2004 |
Methods of Celestial Mechanics: Volume II: Application to Planetary System ... Gerhard Beutler Keine Leseprobe verfügbar - 2004 |